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15 February 2025
 
  » arxiv » 2301.01580

 Article overview



First on-sky results of ERIS at VLT
Kateryna Kravchenko ; Yigit Dallilar ; Olivier Absil ; Alex Agudo Berbel ; Andrea Baruffolo ; Markus J. Bonse ; Alexander Buron ; Yixian Cao ; Angela Cortes ; Felix Dannert ; Richard Davies ; Robert J. De Rosa ; Matthias Deysenroth ; David S. Doelman ; Frank Eisenhauer ; Simone Esposito ; Helmut Feuchtgruber ; Natascha Förster Schreiber ; Xiaofeng Gao ; Hans Gemperlein ; Reinhard Genzel ; Stefan Gillessen ; Christian Ginski ; Adrian M. Glauser ; Andreas Glindemann ; Paolo Grani ; Pierre Haguenauer ; Johannes Hartwig ; Jean Hayoz ; Marianne Heida ; Matthew Kenworthy ; Johann Kolb ; Harald Kuntschner ; Dieter Lutz ; Daizhong Liu ; Mike MacIntosh ; Michaël Marsset ; Gilles Orban de Xivry ; Hakan Özdemir ; Alfio Puglisi ; Sascha P. Quanz ; Christian Rau ; Armando Riccardi ; Daniel Schuppe ; Frans Snik ; Eckhard Sturm ; Linda Tacconi ; William D. Taylor ; Erich Wiezorrek ;
Date 4 Jan 2023
AbstractERIS (Enhanced Resolution Imager and Spectrograph) is a new adaptive optics instrument installed at the Cassegrain focus of the VLT-UT4 telescope at the Paranal Observatory in Chile. ERIS consists of two near-infrared instruments: SPIFFIER, an integral field unit (IFU) spectrograph covering J to K bands, and NIX, an imager covering J to M bands. ERIS has an adaptive optics system able to work with both LGS and NGS. The Assembly Integration Verification (AIV) phase of ERIS at the Paranal Observatory was carried out starting in December 2021, followed by several commissioning runs in 2022. This contribution will describe the first preliminary results of the on-sky performance of ERIS during its commissioning and the future perspectives based on the preliminary scientific results.
Source arXiv, 2301.01580
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